RMS Images are meant to represent the root-mean-square deviation from the mean (rmsd) appropriate to measure the noise level in a Gaussian distribution.

maximum 2.2147e-03 Jy/beam
minimum 1.1275e-04 Jy/beam
mean 1.8691e-04 Jy/beam
median 1.4279e-04 Jy/beam
sigma 9.4116e-05 Jy/beam
MAD rms 1.7323e-05 Jy/beam

RMS images

TSKY0001.sb32522754.eb32557595.57620.02690508102_split.ms

Pilot.ql.Cygnus_e3.J203509_393000.10.2048.v1.I.iter1.image.pbcor.tt0.rms.sky.png

No pipeline QA for this task.
vis
/lustre/aoc/cluster/pipeline/vlass_auto/spool/quicklook/Pilot_Cygnus_e3.J203509+393000_P33692v1_2019_02_07T15_59_53.833/working/TSKY0001.sb32522754.eb32557595.57620.02690508102_split.ms
output_dir
/lustre/aoc/cluster/pipeline/vlass_auto/spool/quicklook/Pilot_Cygnus_e3.J203509+393000_P33692v1_2019_02_07T15_59_53.833/working
Start time
2019-02-10 15:20:47.073
End
2019-02-10 15:22:42.344
Duration
0:01:55.271
Note, WebLog generation is not included in the time.

CASA logs for stage 6